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The Journal of Neuroscience, June 15, 1998, 18(12):4775-4784
Circadian Rhythms of Rod-Cone Dominance in the Japanese
Quail Retina
Mary K.
Manglapus1,
Hiroyuki
Uchiyama2,
Neal F.
Buelow1, and
Robert B.
Barlow1
1 Center for Vision Research, State University of New
York Health Science Center, Syracuse, New York 13210, and
2 Department of Information and Computer Science, Faculty
of Engineering, Kagoshima University, Kagoshima 890, Japan
 |
ABSTRACT |
When the Japanese quail is held in constant darkness, retinal
responses (ERG b-waves) increase during the animal's subjective night
and decrease during its subjective day. Rod photoreceptors dominate the
b-wave responses (
max = 506 nm) to all stimulus intensities at night but only to those intensities below the cone threshold during the day. Above the cone threshold, cones dominate b-wave responses (
max, ~550-600 nm) during the
day regardless of the state of retinal adaptation. Apparently a
circadian oscillator enables cone signals to block rod signals during
the day but not at night. The ERG b-wave reflects the activity of
bipolar cells that are postsynaptic to rods and cones. The ERG a-wave
reflects the activity of both rods and cones. The amplitude of the
isolated a-wave (PIII) changes with time of day, as does that of the
b-wave, but its spectral sensitivity does not. The PIII responses are maximal at ~520 nm both day and night and may reflect multiple receptor mechanisms. The shift in rod-cone dominance detected with the
ERG b-wave resembles the Purkinje shift of human vision but, unlike the
Purkinje shift, does not require a change in ambient light intensity.
The shift occurs in constant darkness, with a period of ~24 hr
indicative of a circadian rhythm in the functional organization of the
retina.
Key words:
circadian rhythm; retina; ERG; quail; rod-cone
dominance; photoreceptor
 |
INTRODUCTION |
Animals can see over wide ranges of
light intensity from sunlit days to starlit nights-more than a
1,000,000-fold change in illumination. In most vertebrate retinas, two
types of photoreceptors, rods and cones, provide visual sensitivity
throughout this range. Rods mediate vision in dim light, whereas cones
operate in bright light and provide color vision. Rods, cones, and the
cells they innervate have important roles in setting the sensitivity of
the retina (Dowling, 1987
). In many animals, the retina adapts in response to changes in ambient illumination; in others, it anticipates them.
For example, a circadian clock in the brain of Limulus
transmits efferent optic nerve activity to the lateral eyes, increasing their sensitivity at night (Barlow et al., 1977
; Barlow, 1988
) and
enabling them to see nearly as well at night as they do during the day
(Powers et al., 1991
; Herzog et al., 1996
). Circadian rhythms have been
detected in numerous invertebrate visual systems but are not unique to
them (Block et al., 1993
). These rhythms characterize many vertebrate
visual systems that possess circadian oscillators in the
suprachiasmatic nucleus, in the pineal gland, and in the eyes
themselves (Hamm and Menaker, 1980
; Besharse and Iuvone, 1983
; Terman
and Terman, 1985
; Remé et al., 1991
) (L. Li and J. E. Dowling, in press).
At the level of the retina, circadian rhythms have been detected in
such cellular and molecular processes as photoreceptor disk shedding
[chick (Young, 1978
); mammals (LaVail and Ward, 1978
)], retinomotor
movements [amphibians (Pierce and Besharse, 1985
); fish (Dearry and
Burnside, 1988
)], enzyme activities [amphibian (Besharse and Iuvone,
1983
)], and gene transcription [chick (Pierce et al., 1993
);
amphibian (Green and Besharse, 1994
)]. Circadian rhythms have also
been reported in the light sensitivity of retinas in mammals
(Brandenburg et al., 1983
; Terman and Terman, 1985
), fish (Bassi and
Powers, 1987
), and birds (Barattini et al., 1981
; Schaeffel et al.,
1991
; Uchiyama et al., 1991
). It is not known whether the rhythms in
cellular and metabolic processes of the retina are related to those in
sensitivity.
Here we report circadian changes in the functional organization of the
quail retina. We show that both photoreceptor (PIII) and
postphotoreceptor (b-wave) responses exhibit circadian rhythms. An
endogenous clock seems to modulate PIII responses by influencing the
sensitivities of both rods and cones. The clock modulates b-wave
responses by shifting the relative weight of rod and cone inputs to the
inner retina. When an animal remains in constant darkness, cones
dominate retinal sensitivity during the day, and rods dominate at
night. Circadian oscillators located in the eyes themselves may control
the circadian rhythms we report here (Underwood et al., 1988
,
1990
).
 |
MATERIALS AND METHODS |
Animal maintenance. Sexually mature Japanese quail
(Coturnix coturnix japonica) were purchased from Bruckner
poultry laboratory (Cornell University, Ithaca, NY) and maintained in a
12/12 hr light/dark cycle at least 1 week before experimentation. Birds were anesthetized initially with an intraperitoneal injection of Rompun
(2 mg/kg) and an intramuscular injection of Ketamine (5 mg/kg). A
tracheotomy was performed, and one caudal thoracic air sac was
punctured to ensure one-way air flow. Animals were then given an
intraperitoneal injection of urethane (10%; 1.0 ml/100 gm body weight)
and an intramuscular injection of curare (0.1%; 0.3-0.4 ml/100 gm
body weight) and placed on moisturized air (95% O2;
5% CO2; 140 ml/min). The bird was then transferred to a stereotactic holder within a light-tight cage. Heart rate was
monitored (Global Specialties oscilloscope; Realistic speakers) via
intramuscular electrodes placed in the breast muscles, and body
temperature was maintained with a heating pad (38-40°C). Animals
were maintained under deep anesthesia with either an intramuscular or
an intraperitoneal infusion of Ringer's solution, urethane (4.0-8.1
mg/hr), curare (0.16-0.32 mg/hr), and glucose (2.5%).
Recording techniques. A teflon-coated silver-chloride wire
(A-M Systems; 0.005" bare) electrode was threaded into a 30 gauge needle and passed through the sclera into the vitreous of each eye. The
experimental eye was sutured open, and the cornea was covered with high
viscosity clear silicone to prevent drying (Dow Corning); the other eye
served as a reference. A light pipe was positioned ~5 mm from the
corneal surface of the experimental eye to ensure full-field
illumination; the reference eye was closed. Stimuli for spectral
sensitivity data were generated with a xenon light source fitted with a
0.125 m, single-grating monochromator and 10 nm bandpass (Oriel
Corporation). For some experiments (see Figs. 6, 7), the unattenuated
output (Log I = 0.0) of the light pipe was
~1014 photons sec
1
cm
2 (Photodiode Model 211; Graseby Optronics).
Flashes delivered from a tungsten source (
= 610 nm) were used for
long-term experiments (see Fig. 3). The light intensities of both light
sources were attenuated by neutral density filters.
Electroretinograms (ERGs) were elicited with a 50 msec flash of light,
amplified (WPI Dam 50; filter settings of 0.1 Hz to 3 kHz), and
recorded on a Gould chart recorder (Gould Model 220) and/or a Hewlett
Packard Signal Averager or Tektronix Oscilloscope (TDS 310). Reducing
flash duration to 10 msec did not significantly alter the shape and/or
amplitude of the ERG b-wave, but extending the duration beyond 50 msec
decreased its amplitude. Figure 1 (top) shows the waveform of an ERG. The corneal positive
b-wave is a convenient measure of retinal sensitivity (Dowling, 1960
). It reflects the responses of ON bipolar cells and thus represents postsynaptic activity in the retina (Stockton and Slaughter, 1989
). The
b-wave amplitude is defined as the voltage difference between the
trough of the a-wave and the peak of the b-wave (Arden et al., 1960
).
The amplitude of the b-wave was tracked for up to 50 hr while animals
were maintained in constant darkness. Throughout the period, light
flashes of constant intensity were delivered once every 10 or 15 min,
alternating between 470 and 610 nm. Spectral sensitivities of the
b-wave responses were measured day and night for wavelengths ranging
from 425 to 700 nm while the animal remained dark-adapted. To improve
the signal-to-noise ratio of responses to low intensity stimuli (Log
I =
4.5 to Log I =
3.0), we averaged up to 100 b-waves. A
criterion response amplitude was established for each experiment in the
range of 40-60 µV, and the intensities (photons
sec
1 cm
2) required to elicit
that response were plotted as a function of wavelength to yield the
spectral sensitivities reported here.

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Figure 1.
ERGs recorded from the Japanese quail eye.
Top, An ERG evoked by a 50 msec flash of light ( = 520 nm). The a-wave amplitude is measured from the baseline to the
trough of the a-wave, and the b-wave amplitude is measured from the
trough of the a-wave to the peak of the b-wave. Bottom,
An ERG after APB was injected in the vitreous to block the b-wave. The
isolated a-wave (PIII) was evoked by a 50 msec
flash of light ( = 520 nm). The photoreceptor response
(PIII) is measured from the baseline to the
bottom of the trough. Each waveform is the average of
eight responses to light flashes of Log I equals 2.0.
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In addition to the b-wave, we also examined the characteristics of the
photoreceptor component of the ERG or PIII that is the isolated a-wave
(Granit, 1947
). The PIII often exhibits two components, fast PIII and
slow PIII, both of which reflect photoreceptor activity (Steinberg et
al., 1991
). We isolated PIII with 2-amino-4-phosphonobutyric acid (APB)
that blocks ON bipolar cell responses, thereby eliminating the b-wave
(Slaughter and Miller, 1981
, 1983
). After ensuring the retina had a
normal ERG, we injected APB into the vitreous (20 mM; 10 µl) under dim red light. Although APB generally blocked the b-wave
within 20 min, the animal was allowed to dark adapt at least 30 min
before testing. PIII amplitude (Fig. 1, bottom) was measured
as the difference between the baseline and the trough of the corneal
negative deflection of the waveform. The PIII was evoked by brief
flashes of light (
= 520 nm) presented every 10 or 15 min for up to
50 hr. We measured the spectral sensitivity of PIII at various times
during the 50 hr period using the same technique described above for
the b-wave but with a lower criterion response (10 µV).
 |
RESULTS |
Retinal sensitivity changes with time of day
Figure 2A displays
ERGs recorded day and night from the dark-adapted quail eye in
situ in response to 520 nm light flashes. At night, the b-wave
amplitude was larger than it was during the day, especially in response
to intermediate and high light intensities. At the highest intensity
flash, the b-wave was 41% higher at night, reaching an amplitude of
105 µV versus 62 µV during the day (Fig. 2A). The
latency of the peak of the b-wave response decreased as intensity
increased but did not change significantly from day to night. It was
minimal at the highest intensity (~40 msec) and maximal at the lowest
intensity (~80 msec). The b-wave is a measure of responses generated
by second order cells in the inner nuclear layer of the retina. Figure
2A shows that the a-wave, which reflects photoreceptor activity, was also greater in amplitude at night. To
study its properties in greater detail, we isolated it by blocking the
b-wave with APB.

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Figure 2.
ERGs recorded in response to a wide range of light
stimuli ( = 520 nm) day and night. A, The ERG b-wave,
which is a postphotoreceptor response, is larger at night than it is
during the day. Light flashes (50 msec) occurred at the beginning of
each trace. B, The PIII component, which is a
photoreceptor response, is also larger at night. Light flashes (50 msec) occurred ~50 msec after the beginning of each trace. Animals
were maintained in constant darkness for all recordings. Oscillatory
potentials are apparent near the peak of the b-wave during the day and
on the falling phase at night. The exact origin of these components of
the b-wave is not known (Dowling, 1987 ).
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Photoreceptor sensitivity changes with time of day
Figure 2B shows isolated a-waves (PIII) recorded
from the dark-adapted quail eye in situ in response to 520 nm light flashes. The PIII component was first detected at Log I equals
3.5. Its amplitude increased with flash intensity and was larger at
night for all test intensities. At the highest intensity (Log I = 0.0), the PIII was 34% larger at night, reaching 170 µV versus a
daytime amplitude of 110 µV (Fig. 2B). Latency to
the peak of the PIII decreased as intensity increased from ~135 msec
at Log I equals
3.5 to ~75 msec at Log I equals 0.0 during the day
and from ~135 msec at Log I equals
3.5 to ~50 msec at night.
The robust change in PIII amplitude with time of day shown in Figure
2B was not observed in every experiment. Most yielded significant changes in PIII amplitude over the first 24 hr period, but
not during the second day in constant darkness when rhythmic changes
were often highly damped or nonexistent. In experiments that did not
isolate the PIII, day-night changes in a-wave amplitude were
occasionally detected as in Figure 2A but were not
seen in most cases (see Fig. 3A). It is not known why the
magnitude of the circadian rhythm of the photoreceptor response varies
from one preparation to the next.
In summary, the results in Figure 2 show that both photoreceptor and
postphotoreceptor components of the ERG change with time of day, high
at night and low during the day. Are these changes indicative of an
endogenous rhythm in retinal function?
A circadian oscillator seems to control day-night changes in
the retina
Figure 3A plots a- and
b-wave responses to 470 nm flashes recorded over a period of 2 d
in constant darkness. The amplitude of the b-wave increases during the
first subjective night, decreases during the following subjective day,
and again increases during the second night. The rhythmic behavior of
the b-wave amplitude is damped with ~60% reduction in maximum
amplitude on the second night relative to the first night. The a-wave
amplitude does not exhibit such rhythmic changes but also does not
remain constant over the 2 d period. It decays slowly after the
beginning of the first subjective night. B-wave responses to 610 nm
flashes (data not shown) also were nonrhythmic and decayed slowly over
the 2 d period. The slow decay of the a- and b-waves over several
days characterizes the majority of our experiments and seems to
represent a gradual decline in retinal sensitivity. Short-term
experiments were more stable, and b-wave responses to 610 nm flashes
did not change with time of day, indicating that 610 nm is an
isosbestic point for b-wave sensitivity (see Fig. 5A). We
used this isosbestic behavior of 610 nm responses to compensate for
long-term changes in retinal sensitivity. For example, Figure
3B plots the ratio of 470 to 610 nm responses as a function
of time of day.

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Figure 3.
ERGs recorded over several days in constant
darkness. A, ERG a- and b-waves in response to 470 nm
flashes are shown. The b-wave amplitude is high during the subjective
night (black bars) and low during the subjective day
(gray bars). After reaching a stable level early
in the experiment, the a-wave amplitude decayed slowly without the
day-night changes exhibited by the b-wave. B-waves in response to
longer wavelength (610 nm) flashes (data not shown) followed the same
time course as the a-wave, indicating a slow loss of retinal
sensitivity over the course of the experiment. B, The
ratio of b-wave amplitude in response to a 470 nm flash to that in
response to a 610 nm flash is shown. Under ideal conditions, b-wave
responses to 610 nm light flashes do not change over the course of the
experiment. The ratio provides a convenient means for normalizing the
data when retinal sensitivity decreases during long-term experiments.
C, A 4 hr delayed entrainment cycle shifts the rhythmic
changes in the b-wave relative to those shown in B. Over
nine experiments, the period of this rhythm ranges from 20 to 28 hr
with an average of 24.4 ± 3.0 hr.
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The light intensity used to track long-term changes in the ERG in
Figure 3A was sufficiently high to evoke a medium amplitude b-wave and a small but discernible a-wave. Because the a-wave did not
change significantly with time of day, it does not interfere with
measurements of the b-wave. In other experiments in which the light
intensity used to track the ERG was too low to evoke a detectable
a-wave, the b-wave exhibited robust day-night rhythms similar to those
shown in Figure 3, B and C. The intensity
required to evoke a measurable a-wave is generally 2 log units greater than that for evoking a detectable b-wave.
Figure 3B plots the ratio of 470 to 610 nm b-wave responses
from the data in Figure 3A. Normalizing the data in this
manner yields nearly equal nighttime increases in retinal sensitivity. After the first night in darkness, retinal sensitivity decreases, reaching its lowest levels during the middle of the second subjective day, and then increases in anticipation of the second subjective night,
reaching peak amplitudes several hours after subjective dusk.
Figure 3C plots the ratio of 470 to 610 nm responses
recorded from an animal exposed to a light/dark entrainment cycle that was shifted by 4 hr with respect to that for the experiment shown in
Figure 3, A and B. Lights were turned on at 6 A.M. and off at 6 P.M. in synchrony with the solar day. Here again the
b-wave is maximal around the middle of the first subjective night
(black bars) and decreases throughout the early morning
hours, with the smallest responses recorded around noon the following
day. These experiments show that the day-night changes in retinal
sensitivity continue in constant darkness and can be entrained to a new
light cycle, two hallmarks of an endogenous circadian rhythm.
The photoreceptor response (PIII) also changes with time of day. In the
experiment shown in Figure 4, an animal
was maintained in constant darkness while the isolated a-wave (PIII)
was recorded continuously over ~48 hr. During the subjective night,
the PIII amplitude grows, reaching peak amplitudes near midnight, and
then declines rapidly to a trough during the subjective day. The PIII amplitude begins to grow again after noon, just before the projected time of sunset. The amplitude of the response does not reach the heights recorded during the first subjective night. Because there is no
isosbestic point for the PIII (see Fig. 5B), we cannot
normalize the data to adjust for long-term decline in the sensitivity
of the preparation, as was done for the b-wave. However, the circadian changes in PIII amplitude are similar to those detected for the unnormalized b-wave data (Fig. 3A). To explore the possible
mechanisms underlying these day-night changes, we measured the
spectral sensitivity of both b-wave and PIII day and night.

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Figure 4.
Photoreceptor responses change with time of day
while an animal remains in constant darkness. In response to a 50 msec
flash ( = 520 nm), the amplitude of the isolated a-wave (PIII)
increases during the subjective night (black bars),
decreases during the subjective day (gray bars),
and again increases during the subjective night.
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Spectral sensitivity changes with time of day
ERG responses to test wavelengths spanning the visible spectrum
were measured in dark-adapted animals day and night (Fig. 5). The spectral sensitivity of the
b-wave shifts from day to night with its amplitude peaking at
intermediate wavelengths (~500 nm; filled circles)
at night and at longer wavelengths (~550-600 nm; open
circles) during the day (Fig. 5A). The smooth
curve is a nomogram for a rod photopigment (
max = 506 nm) based on our microspectrophotometric measurements (see Discussion).
In the vicinity of 610 nm, the spectral sensitivity of the b-wave does not change significantly from day to night, indicating that this is an
isosbestic region. The shift of peak spectral sensitivity to longer
wavelengths during the day is associated with an approximately sixfold
or 0.8 log unit decrease in sensitivity. More than 100-fold decreases
in sensitivity were detected for the responses to shorter wavelength
flashes (
470 nm).

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Figure 5.
Spectral sensitivity of the retina changes with
time of day. A, Spectral sensitivity of the b-wave is
high at night (filled circles;
max, ~500 nm) and low during the day
(open circles; max, ~550-600
nm). Retinal sensitivity does not change with time of day in the region
of 610 nm, which is an isosbestic point. Criterion responses were
40-60 µV for individual experiments (n = 7).
B, Spectral sensitivity of the PIII component also
increases at night but shows no spectral shift
( max, ~520 nm during both day and night).
Criterion responses were 10 µV (n = 3).
C, Changes in b-wave spectral sensitivity of a single
retina over a 2 d period are shown. As in A,
sensitivity is low during the day (open symbols) and
high at night (filled circles). D,
Changes in PIII spectral sensitivity of a single retina during 2 d
in constant darkness are shown. Again, sensitivity is high at night
(filled circles) and low during the day
(open symbols). Day data were taken from 10 A.M. to 3 P.M., and night data are from 8 P.M. to midnight. Solid
curves are rhodopsin nomograms ( max = 506 nm).
Error bars in A indicate SEMs and in B
indicate SDs.
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Figure 5B shows the day and night spectral sensitivities of
photoreceptor responses measured with the APB-isolated a-wave (PIII).
Regardless of time of day, spectral sensitivity of PIII peaks at
~520 nm with the greatest day-night changes occurring at middle
wavelengths. What receptor mechanisms underlie PIII spectral
sensitivity? The 506 nm nomogram for the rod pigment does not fit
either the daytime (open circles) or nighttime data (filled circles) well. This is also the case for a
510 nm nomogram that we derived from our microspectrophotometric
measurements of cones (curve not shown). In view of the variability of
the data, it is not possible to determine whether rods, cones, or their
combination generate the PIII. Generally, avian retinas contain
relatively few rods (Walls, 1963
). In the chicken, rods comprise 14%
of the photoreceptor population in the central retina and just 30% in
the periphery (Morris, 1976
). Assuming that quail has a similar
distribution of photoreceptors, it is not surprising that cones may
contribute to the PIII response. The changes in photoreceptor
sensitivity with time of day measured with PIII do not parallel the
overall changes in retinal sensitivity detected with the b-wave.
Whereas retinal sensitivity decreases and shifts to longer wavelengths
during the day, the photoreceptor response decreases without a
corresponding spectral shift.
The day-night changes in spectral sensitivity of the b-wave and PIII
for individual animals (Fig. 5C,D) match the
average data shown in Figure 5, A and B. During
Day 1, the spectral sensitivity of the b-wave (Fig. 5C)
peaked at long wavelengths (open circles; 550-600 nm) and
appears cone dominated. At night, sensitivity increased (0.8 log units)
and shifted to shorter wavelengths (filled circles;
~500 nm) and appears to be dominated by rod responses. On Day 2, the
retinal sensitivity returned to its low daytime state, with the peak
sensitivity around 600 nm (open squares). This experiment
was repeated for the PIII response in another animal (Fig.
5D). The sensitivity of the PIII response was low during the
day and increased at night (~0.8 log units). During Day 2, its
sensitivity decreased to the Day 1 level. Unlike the b-wave, the
spectral sensitivity of PIII does not shift with time of day.
Amplitude of circadian rhythms depends on stimulus intensity
The growth of the ERG b-wave in Figure 2A
increases monotonically with light intensity at night but not during
the day. Note that during the day, the b-wave amplitude increases with
increasing intensity from Log I equals
4.5 to Log I equals
3.5 but
remains nearly unchanged over the 30-fold increase in light intensity from Log I equals
3.5 to Log I equals
2.0. For intensities greater than Log I equals
1.5, the b-wave again grows monotonically with light intensity. Plotting the ERG amplitude as a function of light intensity (Fig. 6) reveals a dramatic
day-night difference in the behavior of the b-wave, especially at
shorter wavelengths. All daytime intensity-response functions exhibit
a plateau corresponding to b-wave amplitudes in the range of 4 to 8 µV. The plateau is most pronounced at
equals 470 nm and minimal
at
equals 610 nm. The long wavelength part of the spectrum
generally represents an isosbestic region in which day-night changes
in sensitivity are minimal. Unlike daytime responses, the b-wave
increases smoothly at night with light intensity, and the
intensity-response functions generally do not exhibit distinct
plateaus. The slight suggestion in the data of a plateau at 520 nm (Log
I,
3.5 to
3.0) was observed only in this experiment (see Fig.
7).

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Figure 6.
Intensity-response functions of the ERG b-wave
measured day and night in constant darkness. A-D, The
amplitude of the ERG response is plotted as a function of Log I for
four wavelengths. The stimulus intensity at Log I equals 0.0 is
1014 photons sec 1
cm 2 that for a 50 msec flash is 5 × 1012 photons cm 2
flash 1. The intensity-response functions change
with time of day for all wavelengths tested. They grow monotonically
with increasing stimulus intensity at night (filled
circles) but exhibit plateau regions at lower light stimuli
during the day (open circles). The plateaus become less
prominent at longer wavelengths.
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We further explored the plateau region in the intensity-response
function by averaging the results from several experiments for
intermediate light levels (Fig. 7). In
the low to intermediate intensity range (Log I,
4.5 to
2), a
plateau is clear in the daytime responses at short wavelengths (
= 470 nm) and decreases with increasing wavelength until it is
indistinguishable at
equals 610 nm. Although a plateau was
detectable at long wavelengths in the experiment shown in Figure 6,
this is not the case for the averaged data shown in Figure 7. The
averaged nighttime responses grow monotonically with light intensity,
with no clear plateau detectable at any wavelength. Daytime and
nighttime responses nearly overlay at
equals 610 nm, confirming
this to be an isosbestic region for retinal sensitivity. The PIII grows
monotonically with light intensity both day and night for all
wavelength stimuli, i.e., no plateaus are evident. Only the
intensity-response functions of the postsynaptic b-wave response
exhibits this characteristic plateau region.

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Figure 7.
Average intensity-response functions over the
plateau region (n = 3). Data from individual
experiments were scaled vertically to adjust for differences in
sensitivity. As indicated in Figure 6, the plateau in the daytime
function is most prominent at shorter wavelengths ( = 470 nm). It is
not detectable at equals 610 nm, which is an isosbestic point for
most experiments. Error bars give SDs.
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Responses at low light levels do not exhibit robust
circadian rhythms
In Figure 6, responses at low light intensities exhibit little or
no changes from day to night. To explore the possible underlying mechanisms, we analyzed the spectral sensitivity of the dark-adapted retina at both low and high light levels. Figure
8 plots spectral sensitivities of b-wave
responses above and below the cone threshold. At low light intensities,
spectral sensitivity for a criterion of 3 µV is approximately the
same day and night and matches the rhodopsin nomogram
(
max = 506 nm) well. However, at intensities required to
produce a 30 µV response, spectral sensitivity shows distinct
day-night changes, also shown in Figure 5. The rhodopsin nomogram
(
max = 506 nm) matches well the nighttime data
regardless of the criterion level, indicating that nighttime responses
are dominated by rod activity at all stimulus levels. This is not the
case during the day. Spectral sensitivity shifts from rod dominance
(
max = 506 nm) at low light intensities to what appears to be cone dominance (
max, 550-600 nm) at higher
intensities. We conclude that a circadian oscillator does not strongly
influence retinal responses to low intensity stimuli during either the
day or night. Responses to these low intensities are rod-dominated regardless of the time of day.

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Figure 8.
Circadian rhythms in retinal sensitivity are most
prominent above the cone threshold. Sensitivity of the retina below the
cone threshold (criterion = 3 µV) does not change with time of
day and matches a rhodopsin nomogram ( max = 506 nm;
solid line) reasonably well. Sensitivity above the cone
threshold (criterion = 30 µV) is greater at night and is also
well fit by a rhodopsin nomogram ( max = 506 nm).
However, during the day, sensitivity decreases and shifts to longer
wavelengths ( max, ~550 nm) and no longer
matches a rhodopsin nomogram.
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Cones dominate the light-adapted retina regardless of time
of day
Figure 9 plots b-wave spectral
sensitivity day and night in both light- and dark-adapted animals.
During the day, maximal sensitivity was between 550 and 600 nm
regardless of the state of adaptation, indicative of cone dominance
(filled and open circles). Light
adaptation at night reduced sensitivity by ~30-fold and shifted the
peak sensitivity from
max equals 506 nm
(filled squares) to a
max between
~550 and 600 nm (open squares). Light adaptation during
the day decreased b-wave sensitivity by 2.5-fold from the dark-adapted
state but remained cone-dominated. Thus, regardless of time of day, the
sensitivity of the light-adapted retina is cone-dominated. A circadian
clock shifts the retina from cone to rod dominance at night in constant
darkness. However, light adaptation at night can override the clock and
shift the retina to cone dominance.

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Figure 9.
Light adaptation of the retina at night produces a
daytime-like spectral sensitivity. Dark-adapted spectral sensitivity
(filled symbols) exhibits rod dominance at night.
Light adaptation (open symbols) reduces nighttime
sensitivity and shifts peak spectral sensitivity to longer wavelengths
( max, ~550-600 nm). Light adaptation was
achieved by opening the cage to ambient room light. (Daytime light,
n = 2; nighttime light, n = 3;
daytime and nighttime dark data replotted from Fig.
5A).
|
|
 |
DISCUSSION |
Circadian rhythms in the Japanese quail retina
The ERG of the Japanese quail undergoes daily changes in both
photoreceptor (PIII) and retinal (b-wave) sensitivity. These persist
when the animal is held in complete darkness and thus represent
endogenous circadian rhythms. The changes in retinal sensitivity are
more robust, ~100-fold greater, at shorter wavelengths than are those
in photoreceptor sensitivity. The rhythmic changes in the amplitude of
the b-wave depend on both time of day and stimulus intensity, whereas
those in the amplitude of PIII depend only on time of day. These
circadian rhythms may be related to that of melatonin synthesis
controlled by an intraocular oscillator (Underwood et al., 1988
, 1990
).
Recent studies have explored a possible link between the circadian
changes reported here and the retinal neuromodulators that drive these
changes (Kelly et al., 1996
).
Rod and cone contributions to the ERG
What receptor mechanisms generate the PIII response? Figure
5B plots a nomogram for the 506 nm rod pigment as well as
the spectral sensitivity of the PIII response recorded day and night. The nomogram does not fit either the daytime (open circles)
or nighttime (filled circles) data well. Neither does
a 510 nm nomogram derived from our microspectrophotometric measurements
of cones (curve not shown). The substantial variability of the spectral sensitivity values in Figure 5B precludes our making any
firm conclusions regarding the photoreceptor origin of the PIII
response. We note, however, that cones generally outnumber rods in the
avian retina (Walls, 1963
). For example, in the chick retina, cones comprise 86% of the photoreceptors in the central retina and 70% in
the periphery (Morris, 1976
). If quail has a similar photoreceptor distribution, then cones would be expected to contribute to the PIII
response.
What receptor mechanisms generate the b-wave? Figure
10 replots from Figure 5A
the spectral sensitivity of the b-wave measured day and night. The
nighttime data (filled circles) peak in the region of
500 nm, suggesting rod dominance. Preliminary experiments using
microspectrophotometry show that rods in the Japanese quail retina
contain rhodopsin with
max equal to 506 nm (F. Harosi and M. Manglapus, unpublished observations). Figure 5A shows
that a rhodopsin nomogram (
max = 506 nm) fits the data
reasonably well up to 600 nm but not beyond. Higher relative
sensitivity at these long wavelengths suggests that red cones may be
contributing to the ERG b-wave both day and night.
Microspectrophotometric results reveal four different types of cone
pigments and at least three types of oil droplets. The oil droplets act
as cutoff filters to narrow the spectrum of light reaching the cone
pigment. Different oil droplets associate with cones containing
different pigments. Red cones (
max, ~570 nm)
are associated with either red (
max, ~560 nm)
or green (
max, ~440 nm) oil droplets. Combining
spectral properties of the red pigment with that of the red oil droplet yields an absorption spectrum with a
max of ~590 nm
that is nearly identical to that calculated by Bowmaker (1980)
for this
pigment-oil droplet combination (
max = 589 nm) in
pigeon. Combining the spectral properties of rods (
max = 506 nm) with red cones having red oil droplets
(
max, ~590 nm) yields a spectral sensitivity
(Fig. 10, solid line) that fits the nighttime data well.

View larger version (14K):
[in this window]
[in a new window]
|
Figure 10.
Day-night spectral sensitivities can be modeled
with the properties of visual pigments found in the Japanese quail
retina. Nighttime spectral sensitivity of the b-wave (Fig.
5A, filled circles) is fit well by the
solid curve that combines a rod nomogram
( max = 506 nm) with that of a red visual pigment
( max = 570 nm) associated with a red oil droplet
( max = 560 nm). Although the retina is rod-dominated at
night, red cones may contribute to its sensitivity. Daytime spectral
sensitivity (Fig. 5A, open circles) is
fit well by a red visual pigment ( max = 570 nm)
associated with a green oil droplet ( max = 440 nm) that
yields the dotted curve. A red visual pigment associated
with a red oil droplet (dashed curve) does not fit the
daytime sensitivities at middle and short wavelengths well. Other cone
types may contribute to the spectral sensitivity of the retina.
O.D., Oil droplet.
|
|
Can the spectral sensitivity of the daytime state be modeled by pigment
and oil droplet properties measured by microspectrophotometry? The
quail retina contains rods, cones, and double cones. Based on oil
droplet-visual pigment combinations detected with
microspectrophotometry, we generated two spectral sensitivity
functions. One of them (dashed line) combines a nomogram for
a red pigment (
max, ~570 nm) and its red oil
droplet (
max, ~560 nm) and the other
(dotted line) combines a red pigment and green oil droplet
(
max ~440 nm). Note that the red pigment-red oil
droplet combination matches the long wavelength portion of the daytime
spectral sensitivity of the b-wave but not the short wavelength portion
(<570 nm). However, the red pigment-green oil droplet combination
matches the daytime spectral sensitivity well at all wavelengths (Fig.
10). More accurate modeling of the daytime spectral sensitivity will
require further microspectrophotometric analyses as well as more
precise knowledge of the relative abundance of each cone type in the
retina.
Red cones at night?
Red cones can contribute to retinal sensitivity at night only when
stimulus intensities are above the cone threshold. Our best estimate
places human cone threshold in the range of Log I from
5.0 to
4.5.
Cone threshold may be higher in birds because the oil droplets reduce
the maximal pigment absorption by up to 30% (Bowmaker and Knowles,
1977
). We estimate the cone threshold to be Log I
4.0. Figure
8 plots retinal sensitivity for stimulus intensities above and below
the cone threshold. Intensities below the estimated cone threshold
correspond to b-wave amplitudes of 3 µV, whereas intensities above
the cone threshold correspond to amplitudes of 30 µV. The solid
line representing a rhodopsin nomogram (
max = 506 nm) fits the low criterion data reasonably well
(circles) but not the high criterion data
(squares) that exhibit greater sensitivity at long
wavelengths. As described above, a combination of rod and red cone
pigments (Fig. 10, solid line) fits the nighttime data well,
indicating that red cones probably contribute to the nighttime b-wave
response at intensities above the cone threshold. It is interesting
that in goldfish, red cones also contribute to the nighttime spectral
sensitivity of the ERG (Nussdorf and Powers, 1988
) and to cone
horizontal cell responses (Wang and Mangel, 1996
). When the goldfish is
in the dark-adapted nighttime state, the spectral sensitivity of L-type
cone horizontal cells matches that of rod horizontal cells below
max equals 610 nm but not at longer wavelengths where
sensitivity is enhanced 30-fold [see Wang and Mangel (1996)
, their
Fig. 5]. Thus in both goldfish and Japanese quail, red cones seem to
contribute to the sensitivity of the retina at night.
Day-night changes in spectral sensitivity resemble a
Purkinje shift
The shift in spectral sensitivity of the retina (b-wave) to
shorter wavelengths at night is reminiscent of the Purkinje shift in
human vision after dark adaptation. The Purkinje phenomenon in humans
reflects a switch from cone (
max = 550 nm) to rod
(
max = 510 nm) vision. The Purkinje shift in the
Japanese quail does not require a change in background illumination but
persists in constant darkness with rods dominating retinal sensitivity
at night and cones dominating during the day. It seems that a circadian oscillator generates a Purkinje-like shift in the quail retina, adapting it for dim light vision at night.
Cones block rod signals to the inner retina during the day
Although cone threshold is not known in the quail, we estimate
human cone threshold to be in the range of Log I from
5.0 to
4.5 in
our experiments. A plateau in the daytime intensity-response functions
begins ~1 log unit above this level and seems to represent a
transition from rod to cone dominance of retinal sensitivity (Fig. 6).
Below the plateau, rods dominate b-wave responses, whereas above the
plateau, cones do. The plateau extends over ~1.5 log units of light
intensity at
max equals 470 nm and is minimal or barely
detectable at
max > 600 nm where the retinal responses are dominated by cones.
Where in the retina does the clock modulate rod-cone dominance?
Studies in other vertebrates show that the b-wave reflects activity of
ON bipolar cells. Assuming the same is true in the Japanese quail
retina, shifts in rod-cone dominance may occur at or before the
synaptic input to ON bipolar cells. Because there is no significant
rod-cone shift in the photoreceptor-generated PIII (Fig.
5B), cone responses must block rod signals before they reach
the inner retina. This blockade occurs only during the day in the
dark-adapted state. Detection of these rod-cone interactions with ERG
recordings is facilitated by the large complement of cones in the
duplex quail retina. If similar circadian changes occur in the
dark-adapted mammalian retina, they may be obscured by the large
contribution of rods to the ERG.
Circadian rhythms have been reported in the outer retina of other
vertebrates. Rod and cone inputs to the inner retina are modulated by a
circadian clock in fish (Wang and Mangel, 1996
). Light responses of
L-type horizontal cells were studied in intact goldfish retina day and
night. At night, responses of cone horizontal cells resembled those of
rod horizontal cells with regard to waveform, threshold, and spectral
sensitivity (Wang and Mangel, 1996
). During the day, cone-like
responses dominated regardless of the state of adaptation, and the
spectral sensitivity curve closely matches those of red cones. However,
at night when responses were rod-like, light would shift horizontal
cell responses to cone dominance (Wang and Mangel, 1996
). Such results
are strongly reminiscent of those reported here for the Japanese quail
and suggest that circadian clocks and environmental lighting cues
control visual sensitivity by influencing rod and cone pathways in both
species (Wang and Mangel, 1996
).
Xenopus photoreceptors also show modulation of rod-cone
coupling (Witkovsky et al., 1996
). Intracellular rod responses can follow flicker stimulation of >10 Hz by application of a D2
dopaminergic agonist, indicating that rods and cones are coupled by gap
junctions in the photoreceptor layer (Witkovsky et al., 1996
). Recent
evidence suggests that dopamine modulates the rod-cone shifts we
report here (Kelly et al., 1996
).
What retinal cells contain circadian oscillators?
Day-night changes in overall retinal sensitivity measured with
the b-wave are approximately the same as those in photoreceptor sensitivity measured with PIII (Fig. 5), suggesting that circadian rhythms originate in photoreceptors. Analysis of
photoreceptor-generated a-waves recorded from rabbit and
Anolis has not revealed circadian rhythms (Brandenburg
et al., 1983
; Fowlkes et al., 1984
), but such rhythms, if they exist,
may have been masked by the b-wave. However, the excised
Xenopus retina stripped of all neural elements except
photoreceptors exhibits rhythmic synthesis of melatonin, indicating
that the underlying circadian oscillators reside in the photoreceptors
(Cahill and Besharse, 1992
). The quail retina in situ also
synthesizes melatonin rhythmically and does so independently of the
fellow retina (Underwood et al., 1988
), indicating that each retina
possesses independent circadian oscillators. The cellular location of
the oscillators is not known.
Rod-cone shifts in other avian systems
Diurnal changes in avian retinal sensitivity were first identified
by Barattini et al. (1981)
. The spectral sensitivities they report for
pigeon are similar to those we report here for the Japanese quail. Both
reveal a rod-cone shift from day to night. Pigeons show increased
sensitivity at night with a shift toward short wavelength stimuli with
an isosbestic point at
max equals 590 nm (Barattini et
al., 1981
). Although Barattini et al. (1981)
did not comment on changes
in intensity-response functions at various wavelengths, they suggest
that a circadian clock may control the way in which photoreceptors or
postsynaptic elements analyze light and that cones may yield to rod
dominance at night. In a later study, Schaeffel et al. (1991)
measured
the spectral sensitivity of the dark-adapted ERG in chickens at various
times of the day and night. Animals tested at night exhibited a
rod-dominated retina, and those tested during the day exhibited a
cone-dominated retina. Although the day-night spectral sensitivities
they report in chicken resemble those reported here for quail, it is
difficult to reconcile these changes in spectral sensitivity with the
intensity-response functions they report. Specifically, the amplitude
of the criterion response (60 µV) they used to measure spectral
sensitivity does not change from day to night [see Schaeffel et al.
(1991)
, their Fig. 7].
Role of circadian clocks in vision
Although we have noted the existence of circadian rhythms in
avian, fish, and amphibian retinas, they are also prevalent in species
ranging from horseshoe crabs to humans. In some cases the role of
circadian rhythmicity is clear; in others it is not. For example, a
circadian clock in the Limulus brain changes the structure
and function of the retina, increasing its sensitivity at night and
allowing the animal to see mates at night as well as it does during the
day (Barlow et al., 1977
, 1989
; Powers et al., 1991
; Herzog et al.,
1996
; Passaglia et al., 1997
). Ocular clocks have been detected in
several marine mollusks, but their role in vision is not clear (Block
et al., 1993
). Vertebrates such as rabbit and Anolis exhibit
circadian rhythms in retinal sensitivity (Brandenburg et al., 1983
;
Fowlkes et al., 1984
), and the rat exhibits a rhythm in visual
sensitivity (Terman and Terman, 1985
). Also, circadian changes in human
visual sensitivity have been detected (Bassi and Powers, 1986
; Barlow
et al., 1997
).
 |
FOOTNOTES |
Received Sept. 29, 1997; revised March 26, 1998; accepted April 1, 1998.
This research was supported in part by National Institutes of Health
Grant EY 00667 and National Science Foundation Grant IBN 9696208 to
R.B.B. We thank Dr. Mary Pierce for critical reading of this
manuscript.
Correspondence should be addressed to Dr. Mary K. Manglapus, Center for
Vision Research, State University of New York Health Science Center,
750 East Adams Street, Syracuse, NY 13210.
 |
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4132 - 4141.
[Abstract]
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